Early evolution of Quark-Nova Ejecta: Application to Gamma-Ray Bursts

Details Early evolution of Quark-Nova Ejecta: Application to Gamma-Ray Bursts Early evolution of Quark-Nova Ejecta: Application to Gamma-Ray Bursts

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1133..103l&link_type=abstract

GAMMA-RAY BURST: Sixth Huntsville Symposium. AIP Conference Proceedings, Volume 1133, pp. 103-105 (2009).

Physics

Gamma-Ray Sources, Gamma-Ray Bursts, Plasma Reactions, Supernovae

Scientific paper

We explore the dynamical and thermal evolution of the iron-rich ejecta in a Quark-Nova explosion and find that the ejecta breaks up into multiple chunks. If the quark-nova occurs inside a collapsar, the interaction between these chunks and the collapsar envelope leads to features indicative of those observed in Gamma Ray Bursts. These features include: (i) precursor activity (optical, X-ray, γ-ray), (ii) prompt γ-ray emission, and (iii) afterglow emission.

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